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HD 103236


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관련 글

Interstellar polarization at high galactic latitudes from distant stars. VI. Extended polarization map and connection with the local spiral structure.
We present new interstellar polarization measurements for 116 stars athigh galactic latitudes. Our data show that Markkanen's cloud -- themain polarization structure seen in the North Galactic Pole area (b >75 degr) extends further towards lower latitudes. Especially, we havefound a new dust formation in the area 35 degr < l < 45 degr, 57degr < b < 63 degr. Interstellar polarization in this part of thesky peaks at 0.7%, which gives a lower limit to the extinctionAV > 0.23m. Polarization vectors in this cloud are verywell aligned along the direction of l = 50 degr. On the IRAS 100 micronmap this dust structure shows up as a bright emission area. We discussthe new polarization map extending from circumpolar to lower latitudesand point out features which suggest that Markkanen's cloud may be apart of the dust lane in the inner edge of the local spiral or spur.

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관측 및 측정 데이터

별자리:사자자리
적경:11h53m25.11s
적위:+15°59'00.5"
가시등급:8.841
거리:196.078 파섹
적경상의 고유운동:-6.2
적위상의 고유운동:13.8
B-T magnitude:9.519
V-T magnitude:8.897

천체목록:
일반명   (Edit)
HD 1989HD 103236
TYCHO-2 2000TYC 1441-1596-1
USNO-A2.0USNO-A2 1050-06603254
HIPHIP 57969

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